QUANTUM-THEORY OF DILATON GRAVITY IN 1+1 DIMENSIONS

被引:23
作者
HAMADA, KJ
机构
[1] Institute of Physics, University of Tokyo, Meguro-ku, Tokyo, 153, Komaba
关键词
D O I
10.1016/0370-2693(93)91340-S
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the quantum theory of 1 + 1 dimensional dilaton gravity, which is an interesting model with features analogous to the spherically symmetric gravitational systems in 3 + 1 dimensions. The functional measures over the metrics and the dilaton field are explicitly evaluated and the diffeomorphism invariance is completely fixed in the conformal gauge by using the technique developed in two dimensional quantum gravity. We derive the Wheeler-DeWitt like equations as physical state conditions. In the ADM formalism the measures of fields are very ambiguous, but in our formalism they are explicitly defined. A singularity appears at psi2 = kappa(> 0), where kappa = 1/12 (N - 51/2) and N is the number of matter fields. The final stage of the black hole evaporation corresponds to the region psi2 approximately kappa, where the Liouville term becomes important, which just comes from the measure of the metrics. If kappa < 0, the singularity disappears.
引用
收藏
页码:322 / 329
页数:8
相关论文
共 29 条
[21]   FRACTAL STRUCTURE OF 2D - QUANTUM-GRAVITY [J].
KNIZHNIK, VG ;
POLYAKOV, AM ;
ZAMOLODCHIKOV, AB .
MODERN PHYSICS LETTERS A, 1988, 3 (08) :819-826
[22]   WARD IDENTITIES IN 2-DIMENSIONAL GRAVITY [J].
POLCHINSKI, J .
NUCLEAR PHYSICS B, 1991, 357 (01) :241-270
[23]  
POLCHINSKI J, 1990, 1990 P STRING COLL S
[24]  
RUSSO J, SUITP924 STANF U PRE
[25]  
SEIBERG N, 1990, PROG THEORY PHYS S, V102, P319
[26]  
STROMINGER A, UCSBTH9218 PREPR
[27]   HAWKING RADIATION AND BACK-REACTION [J].
SUSSKIND, L ;
THORLACIUS, L .
NUCLEAR PHYSICS B, 1992, 382 (01) :123-147
[28]   SPHERICALLY SYMMETRIC-SYSTEMS OF FIELDS AND BLACK-HOLES .1. DEFINITION AND PROPERTIES OF APPARENT HORIZON [J].
THOMI, P ;
ISAAK, B ;
HAJICEK, P .
PHYSICAL REVIEW D, 1984, 30 (06) :1168-1177
[29]   EVAPORATING BLACK-HOLES IN QUANTUM-GRAVITY [J].
TOMIMATSU, A .
PHYSICS LETTERS B, 1992, 289 (3-4) :283-286